Zobrazeno 1 - 10
of 29
pro vyhledávání: '"Edelmann, Philipp"'
The cores of main sequence intermediate- and high-mass stars are convective. Mixing at the radiative-convective boundary, waves excited by the convection, and magnetic fields generated by convective dynamos all influence the main sequence and post-ma
Externí odkaz:
http://arxiv.org/abs/2307.15730
Autor:
Bowman, Dominic M., Burssens, Siemen, Pedersen, May G., Johnston, Cole, Aerts, Conny, Buysschaert, Bram, Michielsen, Mathias, Tkachenko, Andrew, Rogers, Tamara M., Edelmann, Philipp V. F., Ratnasingam, Rathish P., Simón-Díaz, Sergio, Castro, Norberto, Moravveji, Ehsan, Pope, Benjamin J. S., White, Timothy R., De Cat, Peter
Publikováno v:
Nature Astronomy, 2019
Almost all massive stars explode as supernovae and form a black hole or neutron star. The remnant mass and the impact of the chemical yield on subsequent star formation and galactic evolution strongly depend on the internal physics of the progenitor
Externí odkaz:
http://arxiv.org/abs/1905.02120
Autor:
Tkachenko, Andrew, Aerts, Conny, Bowman, Dominic M., Van Reeth, Timothy, De Ridder, Joris, Johnston, Cole Campbell, Pedersen, May Gade, Burssens, Siemen, Michielsen, Mathias, Mombarg, Joey, Sekaran, Sanjay, Bjorklund, Robin, Rogers, Tamara, Edelmann, Philipp, Ratnasingam, Rathish Previn, Zwintz, Konstanze, Kollmeier, Juna, Johnson, Jennifer, Rix, Hans-Walter, Tayar, Jamie
The evolution of a star is driven by the physical processes in its interior making the theory of stellar structure and evolution the most crucial ingredient for not only stellar evolution studies, but any field of astronomy which relies on the yields
Externí odkaz:
http://arxiv.org/abs/1903.09205
Autor:
Edelmann, Philipp V. F., Roepke, Friedrich K., Hirschi, Raphael, Georgy, Cyril, Jones, Samuel
Publikováno v:
A&A 604, A25 (2017)
The treatment of mixing processes is still one of the major uncertainties in 1D stellar evolution models. This is mostly due to the need to parametrize and approximate aspects of hydrodynamics in hydrostatic codes. In particular, the effect of hydrod
Externí odkaz:
http://arxiv.org/abs/1704.06261
Autor:
Barsukow, Wasilij, Edelmann, Philipp V. F., Klingenberg, Christian, Miczek, Fabian, Roepke, Friedrich K.
Based on the Roe solver a new technique that allows to correctly represent low Mach number flows with a discretization of the compressible Euler equations was proposed in Miczek et al.: New numerical solver for flows at various mach numbers. A&A 576,
Externí odkaz:
http://arxiv.org/abs/1612.03910
Autor:
Hammer, Nicolay, Jamitzky, Ferdinand, Satzger, Helmut, Allalen, Momme, Block, Alexander, Karmakar, Anupam, Brehm, Matthias, Bader, Reinhold, Iapichino, Luigi, Ragagnin, Antonio, Karakasis, Vasilios, Kranzlmüller, Dieter, Bode, Arndt, Huber, Herbert, Kühn, Martin, Machado, Rui, Grünewald, Daniel, Edelmann, Philipp V. F., Röpke, Friedrich K., Wittmann, Markus, Zeiser, Thomas, Wellein, Gerhard, Mathias, Gerald, Schwörer, Magnus, Lorenzen, Konstantin, Federrath, Christoph, Klessen, Ralf, Bamberg, Karl-Ulrich, Ruhl, Hartmut, Schornbaum, Florian, Bauer, Martin, Nikhil, Anand, Qi, Jiaxing, Klimach, Harald, Stüben, Hinnerk, Deshmukh, Abhishek, Falkenstein, Tobias, Dolag, Klaus, Petkova, Margarita
Publikováno v:
Advances in Parallel Computing, vol. 27: Parallel Computing: On the Road to Exascale, eds. G.R. Joubert et al., p. 827, 2016
In spring 2015, the Leibniz Supercomputing Centre (Leibniz-Rechenzentrum, LRZ), installed their new Peta-Scale System SuperMUC Phase2. Selected users were invited for a 28 day extreme scale-out block operation during which they were allowed to use th
Externí odkaz:
http://arxiv.org/abs/1609.01507
Autor:
Jones, Samuel, Roepke, Friedrich K., Pakmor, Ruediger, Seitenzahl, Ivo R., Ohlmann, Sebastian T., Edelmann, Philipp V. F.
Publikováno v:
A&A 593, A72 (2016)
In the classical picture, electron-capture supernovae and the accretion-induced collapse of oxygen-neon white dwarfs (ONeWDs) undergo an oxygen deflagration phase before gravitational collapse produces a neutron star (NS). These types of core collaps
Externí odkaz:
http://arxiv.org/abs/1602.05771
Akademický článek
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Autor:
Liu, Zheng-Wei, Pakmor, Ruediger, Seitenzahl, Ivo, Hillebrandt, Wolfgang, Kromer, Markus, Roepke, Friedrich, Edelmann, Philipp, Taubenberger, Stefan, Maeda, Keiichi, Wang, Bo, Han, Zhanwen
In the version of the SD scenario of SNe Ia studied here, a CO WD explodes close to the Chandrasekhar limit after accreting material from a non-degenerate He companion. In the present study, we employ the Stellar GADGET code to perform 3D hydrodynami
Externí odkaz:
http://arxiv.org/abs/1307.5579
Autor:
Liu, Zheng-Wei, Pakmor, Ruediger, Roepke, Friedrich K., Edelmann, Philipp, Hillebrandt, Wolfgang, Kerzendorf, Wolfgang E., Wang, Bo, Han, Zhan-Wen
In the SD scenario of SNe Ia the companion survives the SN explosion and thus should be visible near the center of the SN remnant and may show some unusual features. A promising approach to test progenitor models of SNe Ia is to search for the compan
Externí odkaz:
http://arxiv.org/abs/1303.2691